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| Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 17
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First-Order Line Spread Functions
Table 13.40: Spectral Resolution for CCD First- Order Modes
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Slit
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Spectral Resolution (FWHM in pixels)
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Point Source
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Extended
Source
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3200 Å
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5500 Å
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7000 Å
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10000 Å
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52X0.05 |
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52X0.1 |
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52X0.2 |
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52X0.5 |
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52X2 |
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Figure 13.89: CCD First-Order L-Mode Line Spread Functions

Table 13.41: Spectral Resolution for MAMA First Order Modes
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Slit
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Spectral Resolution (FWHM in pixels)
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Point Source
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Extended
Source
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1200 Å
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1500 Å
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1700 Å
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2400 Å
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52X0.05 |
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52X0.1 |
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52X0.2 |
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52X0.5 |
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52X2 |
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1FWHM with FUV-MAMA (G140L, G140M). 2FWHM with NUV-MAMA (G230L, G230M).
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Figure 13.90: MAMA First-Order Line Spread Functions. Top G140L and G140M, bottom G230L and G230M

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